01 January 1970 4 5K Report

I asked a question in the thread of

https://www.researchgate.net/post/An_old_question_that_is_still_fresh_Is_gravity_a_Newtonian_force_or_Einstein_space-time_curvature/448

I'd like to repost it here:

Stage 1:

Imagine a pair of proton and electron, i.e. a hydrogen atom travels in space. The electron is orbiting classically (gyroscope) or quantumly (combination of random gyroscopes) around the proton. Then a beam of light strikes the pair, and one photon is absorbed.

Say the photon is from a source traveling the same speed and direction as the hydrogen atom (resting frame), then it is easy that we can imagine that the energy is absorbed by the electron and makes the electron orbiting radius larger and rotation speed slower, i.e. with a bigger internal angular momentum but no speeding up as a pair because we "all believe" that photon has no mass. After a while, the electron will relax back to its ground state by emitting a series of lower-energy photons or one photon with the same energy. The angle does matter because the emitted photon seems to carry momentum and leave a push to the hydrogen in the opposite direction of the emission. This is the way I think will satisfy the observation of the solar sail problem when the material needs to be reflective and seems all photon momentum is used to create the solar pressure from the equation I pulled out from readings. Let's assume this emitted photon now strangely carries momentum although I don't see what is the difference between it and the absorbed parent.

Now my questions are,

  • what is the mass of the hydrogen atom when it absorbs the photon and has not speeded up? Note the electron of the atom has a slower rotation speed, larger radius, and bigger angular momentum.
  • what is the mass of the hydrogen atom when it has emitted the absorbed photon and speeded up?
  • is the total energy conserved in this case?
  • is the total mass conserved in this case?
  • is the total momentum conserved in this case?
  • is the total angular momentum conserved in this case?

Stage 2:

Now there is a pair of electron and proton moving away from us say at half the speed of light. This situation naturally occurs in the universe on the stars moving away from us or we can speed up ourselves and observe the atom stay still on Earth. And a beam of light hit it from behind and a photon gets absorbed. At a short moment, the hydrogen atom emits a photon to us and accelerates. Now repeat the above questions and adding one at the last, namely,

  • What is the mass of hydrogen atom at the beginning?
  • What is the mass of the atom after absorbing the photon?
  • what is the mass of the atom after emission?
  • Is mass conserved
  • is energy conserved
  • is momentum conserved
  • is angular momentum conserved
  • are the two photons the same as the two when still?

Because mathematically gravity has some similarity, the question can be pushing the solar system.

Stage 3:

The same as stage 2 but now move towards us.

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